- [1]
R. Penrose, Riv. Nuovo Cim.,1: 252 (1969) [Gen. Rel. Grav.,34: 1141 (2002)]. doi:10.1023/A:1016578408204
- [2]
D. Christodoulou, Phys. Rev. Lett.,25: 1596 (1970)
- [3]
J. M. Bardeen, Nature,226: 64 (1970)
- [4]
D. Christodoulou and R. Ruffini, Phys. Rev. D,4: 3552 (1971)
- [5]
J. D. Bekenstein, Lett. Nuovo Cim.,4: 737 (1972)
- [6]
J. D. Bekenstein, Phys. Rev. D,7: 2333 (1973)
- [7]
J. M. Bardeen, B. Carter, and S. W. Hawking, Commun. Math. Phys.,31: 161 (1973)
- [8]
S. W. Hawking, Commun. Math. Phys.,43: 199 (1975) Erratum: [Commun. Math. Phys.,46: 206 (1976)] doi:10.1007/ BF02345020, 10.1007/BF01608497
- [9]
J. M. Maldacena, Int. J. Theor. Phys.,38: 1113 (1999) [Adv. Theor. Math. Phys.,2: 231 (1998)] doi:10.1023/ A:1026654312961,10.4310/ATMP.1998.v2.n2.a1[hep-th/9711200].
- [10]
S. W. Hawking and D. N. Page, Commun. Math. Phys.,87: 577 (1983)
- [11]
E. Witten, Adv. Theor. Math. Phys.,2: 505 (1998), arXiv:hep-th/9803131
- [12]
A. Chamblin, R. Emparan, C. V. Johnsonet al., Phys. Rev. D,60: 064018 (1999), arXiv:hep-th/9902170
- [13]
A. Chamblin, R. Emparan, C. V. Johnsonet al., Phys. Rev. D,60: 104026 (1999), arXiv:hep-th/9904197
- [14]
M. M. Caldarelli, G. Cognola, and D. Klemm, Class. Quant. Grav.,17: 399 (2000), arXiv:hepth/9908022
- [15]
R. G. Cai, Phys. Rev. D,65: 084014 (2002), arXiv:hep-th/0109133
- [16]
D. Kubiznak and R. B. Mann, JHEP,1207: 033 (2012), arXiv:1205.0559[hep-th
- [17]
D. Kastor, S. Ray, and J. Traschen, Class. Quant. Grav.,26: 195011 (2009), arXiv:0904.2765[hep-th
- [18]
B. P. Dolan, Class. Quant. Grav.,28: 235017 (2011), arXiv:1106.6260[gr-qc
- [19]
S. Gunasekaran, R. B. Mann, and D. Kubiznak, JHEP,1211: 110 (2012), arXiv:1208.6251[hep-th
- [20]
S. W. Wei and Y. X. Liu, Phys. Rev. D,87(4): 044014 (2013), arXiv:1209.1707[gr-qc
- [21]
R. G. Cai, L. M. Cao, L. Liet al., JHEP,1309: 005 (2013), arXiv:1306.6233[gr-qc
- [22]
W. Xu and L. Zhao, Phys. Lett. B,736: 214 (2014), arXiv:1405.7665[gr-qc
- [23]
A. M. Frassino, D. Kubiznak, R. B. Mannet al., JHEP,1409: 080 (2014), arXiv:1406.7015[hep-th
- [24]
R. A. Hennigar, W. G. Brenna, and R. B. Mann, JHEP,1507: 077 (2015), arXiv:1505.05517[hep-th
- [25]
P. Wang, H. Wu, and H. Yang, JCAP,1904: 052 (2019), arXiv:1808.04506[gr-qc
- [26]
R. Wald, Ann. Phys.,82: 548 (1974)
- [27]
V. E. Hubeny, Phys. Rev. D,59: 064013 (1999), arXiv:gr-qc/9808043
- [28]
T. Jacobson and T. P. Sotiriou, Phys. Rev. Lett.,103: 141101 (2009), arXiv:0907.4146[gr-qc
- [29]
A. Saa and R. Santarelli, Phys. Rev. D,84: 027501 (2011), arXiv:1105.3950[gr-qc
- [30]
S. Hod, Phys. Rev. Lett.,100: 121101 (2008), arXiv:0805.3873[gr-qc
- [31]
E. Barausse, V. Cardoso, and G. Khanna, Phys. Rev. Lett.,105: 261102 (2010), arXiv:1008.5159[grqc
- [32]
E. Barausse, V. Cardoso, and G. Khanna, Phys. Rev. D,84: 104006 (2011), arXiv:1106.1692[gr-qc
- [33]
P. Zimmerman, I. Vega, E. Poissonet al., Phys. Rev. D,87(4): 041501 (2013), arXiv:1211.3889[gr-qc
- [34]
M. Colleoni and L. Barack, Phys. Rev. D,91: 104024 (2015), arXiv:1501.07330[gr-qc
- [35]
M. Colleoni, L. Barack, A. G. Shahet al., Phys. Rev. D,92(8): 084044 (2015), arXiv:1508.04031[gr-qc
- [36]
G. E. A. Matsas and A. R. R. da Silva, Phys. Rev. Lett.,99: 181301 (2007), arXiv:0706.3198[gr-qc
- [37]
M. Richartz and A. Saa, Phys. Rev. D,78: 081503 (2008), arXiv:0804.3921[gr-qc
- [38]
S. Isoyama, N. Sago, and T. Tanaka, Phys. Rev. D,84: 124024 (2011), arXiv:1108.6207[gr-qc
- [39]
S. Gao and Y. Zhang, Phys. Rev. D,87(4): 044028 (2013), arXiv:1211.2631[gr-qc
- [40]
S. Hod, Phys. Rev. D,87(2): 024037 (2013), arXiv:1302.6658[gr-qc
- [41]
K. Düzta and. Semiz, Phys. Rev. D,88(6): 064043 (2013), arXiv:1307.1481[gr-qc
- [42]
H. M. Siahaan, Phys. Rev. D,93(6): 064028 (2016), arXiv:1512.01654[gr-qc
- [43]
J. Natario, L. Queimada, and R. Vicente, Class. Quant. Grav.,33(17): 175002 (2016), arXiv:1601.06809[gr-qc
- [44]
K. Düzta, Phys. Rev. D,94(12): 124031 (2016), arXiv:1701.07241[gr-qc
- [45]
K. S. Revelar and I. Vega, Phys. Rev. D,96(6): 064010 (2017), arXiv:1706.07190[gr-qc
- [46]
J. Sorce and R. M. Wald, Phys. Rev. D,96(10): 104014 (2017), arXiv:1707.05862[gr-qc
- [47]
V. Husain and S. Singh, Phys. Rev. D,96(10): 104055 (2017), arXiv:1709.02395[gr-qc
- [48]
T. Crisford, G. T. Horowitz, and J. E. Santos, Phys. Rev. D,97(6): 066005 (2018), arXiv:1709.07880[hep-th
- [49]
B. Gwak, JHEP,1711: 129 (2017), arXiv:1709.08665[gr-qc
- [50]
J. An, J. Shan, H. Zhanget al., Phys. Rev. D,97(10): 104007 (2018), arXiv:1711.04310[hep-th
- [51]
B. Ge, Y. Mo, S. Zhaoet al., Phys. Lett. B,783: 440 (2018), arXiv:1712.07342[hep-th
- [52]
T. Y. Yu and W. Y. Wen, Phys. Lett. B,781: 713 (2018), arXiv:1803.07916[gr-qc
- [53]
B. Gwak, JHEP,1809: 081 (2018), arXiv:1807.10630[gr-qc
- [54]
Y. Gim and B. Gwak, Phys. Lett. B,794: 122 (2019), arXiv:1808.05943[gr-qc
- [55]
D. Chen, Chin. Phys. C,44(1): 015101 (2020), arXiv:1812.03459[gr-qc
- [56]
X. X. Zeng and H. Q. Zhang,Thermodynamics and weak cosmic censorship conjecture in Born-Infeldanti-de Sitter black holes, arXiv: 1901.04247[hep-th]
- [57]
D. Chen, W. Yang, and X. Zeng, Nucl. Phys. B,946: 114722 (2019), arXiv:1901.05140[hep-th
- [58]
B. Gwak, JCAP,1908: 016 (2019), arXiv:1901.05589[grqc
- [59]
X. X. Zeng, Y. W. Han, and D. Y. Chen, Chin. Phys. C,43(10): 105104 (2019), arXiv:1901.08915[gr-qc
- [60]
D. Chen, Eur. Phys. J. C,79(4): 353 (2019), arXiv:1902.06489[hep-th
- [61]
P. Wang, H. Wu, and H. Yang, Eur. Phys. J. C,79(7): 572 (2019)
- [62]
X. X. Zeng, X. Y. Hu, and K. J. He, Nucl. Phys. B,949: 114823 (2019), arXiv:1905.07750[hep-th
- [63]
W. Hong, B. Mu, and J. Tao, Nucl. Phys. B,949: 114826 (2019), arXiv:1905.07747[gr-qc
- [64]
T. T. Hu, Y. Song, S. Sunet al., Eur. Phys. J. C,80(2): 147 (2020), arXiv:1906.00235[hep-th
- [65]
S. Q. Hu, Y. C. Ong, and D. N. Page, Phys. Rev. D,100(10): 104022 (2019), arXiv:1906.05870[gr-qc
- [66]
B. Mu and J. Tao,Minimal Length Effect on Thermodynamics and Weak Cosmic Censorship Conjecture in anti-de Sitter Black Holes via Charged Particle Absorption, arXiv: 1906.10544[gr-qc]
- [67]
K. J. He, X. Y. Hu, and X. X. Zeng, Chin. Phys. C,43(12): 125101 (2019), arXiv:1906.10531[gr-qc
- [68]
Q. Gan, G. Guo, P. Wanget al., Phys. Rev. D,100(12): 124009 (2019), arXiv:1907.04466[hep-th
- [69]
X. X. Zeng and X. Y. Hu,Thermodynamics and weak cosmic censorship conjecture with pressure in the rotating BTZ black holes, arXiv: 1908.03845[gr-qc]
- [70]
K. J. He, G. P. Li, and X. Y. Hu, Eur. Phys. J. C,80(3): 209 (2020), arXiv:1909.09956[hep-th
- [71]
S. Q. Hu, B. Liu, X. M. Kuanget al.,Revisiting Black Hole Thermodynamics in Massive Gravity: Charged Particle Absorption and Shell of Dust Falling, arXiv: 1910.04437 [gr-qc]
- [72]
B. Gwak, JCAP,2003(03): 058 (2020), arXiv:1910.13329[gr-qc
- [73]
Q. Gan, P. Wang, H. Wuet al.,Strong Cosmic Censorship for a Scalar Field in an EinsteinMaxwell-Gauss-Bonnet-de Sitter Black Hole, arXiv: 1911.10996[gr-qc]
- [74]
W. Hong, B. Mu, and J. Tao,Test the Weak Cosmic Censorship Conjecture in Torus-Like Black Hole under Charged Scalar Field, arXiv: 2001.09008[physics.gen-ph]
- [75]
B. Gwak,Thermodynamics in Rotating Anti-de Sitter Black Holes with Massive Scalar Field in Three Dimensions, arXiv: 2002.09729 [gr-qc]
- [76]
P. Wang, H. Wu, and S. Ying,Validity of Thermodynamic Laws and Weak Cosmic Censorship for AdS Black Holes and Black Holes in a Cavity, arXiv: 2002.12233[gr-qc]
- [77]
Y. Zhang and S. Gao, Int. J. Mod. Phys. D,23: 1450044 (2014), arXiv:1309.2027[gr-qc
- [78]
D. Glavan and C. Lin, Phys. Rev. Lett.,124(8): 081301 (2020), arXiv:1905.03601[gr-qc
- [79]
H. Lu and Y. Pang,Horndeski Gravity asD→ 4 Limit of Gauss-Bonnet,arXiv: 2003.11552[gr-qc]
- [80]
W. Y. Ai,A note on the novel 4D Einstein-Gauss-Bonnet gravity, arXiv: 2004.02858[gr-qc]
- [81]
P. G. S. Fernandes,Charged Black Holes in AdS Spaces in 4DEinstein Gauss-Bonnet Gravity, arXiv: 2003.05491[gr-qc]
- [82]
K. Hegde, A. Naveena Kumara, C. L. A. Rizwanet al.,Thermodynamics, Phase Transition and Joule Thomson Expansion of novel 4-D Gauss Bonnet AdS Black Hole, arXiv: 2003.08778 [gr-qc]
- [83]
D. V. Singh and S. Siwach,Thermodynamics and P-v criticality of Bardeen-AdS Black Hole in 4-D Einstein-Gauss-Bonnet Gravity, arXiv: 2003.11754[gr-qc]
- [84]
S. A. Hosseini Mansoori,Thermodynamic geometry of novel 4-D Gauss Bonnet AdS Black Hole, arXiv: 2003.13382[gr-qc]
- [85]
S. W. Wei and Y. X. Liu,Extended thermodynamics and microstructures of four-dimensional charged Gauss-Bonnet black hole in AdS space, arXiv: 2003.14275[gr-qc]
- [86]
B. Eslam Panah and K. Jafarzade,4D Einstein-Gauss-Bonnet AdS Black Holes as Heat Engine, arXiv: 2004.04058[hep-th]
- [87]
R. A. Konoplya and A. F. Zinhailo,Quasinormal modes, stability and shadows of a black hole in the novel 4D Einstein-Gauss-Bonnet gravity, arXiv: 2003.01188[gr-qc]
- [88]
R. A. Konoplya and A. Zhidenko,(In)stability of black holes in the 4D Einstein-Gauss-Bonnet and EinsteinLovelock gravities, arXiv: 2003.12492[gr-qc]
- [89]
S. L. Li, P. Wu, and H. Yu,Stability of the Einstein Static Universe in 4D Gauss-Bonnet Gravity, arXiv: 2004.02080[gr-qc]
- [90]
C. Y. Zhang, S. J. Zhang, P. C. Liet al.,Superradiance and stability of the novel 4D charged Einstein-Gauss-Bonnet black hole, arXiv: 2004.03141[gr-qc]
- [91]
A. K. Mishra,Quasinormal modes and Strong Cosmic Censorship in the novel 4D Einstein-Gauss-Bonnet gravity, arXiv: 2004.01243[gr-qc]
- [92]
S. Hendi, S. Panahiyan, and M. Momennia, Int. J. Mod. Phys. D,25(06): 1650063 (2016), arXiv:1503.03340[gr-qc
- [93]
S. H. Hendi, G. Q. Li, J. X. Moet al., Eur. Phys. J. C,76(10): 571 (2016), arXiv:1608.03148[gr-qc
- [94]
S. Hendi, B. Panah, and S. Panahiyan, Fortsch. Phys.,66(3): 1800005 (2018), arXiv:1708.02239[hep-th
- [95]
B. Mu, P. Wang, and H. Yang, Adv. High Energy Phys.,2017: 3191839 (2017), arXiv:1408.5055[gr-qc
- [96]
J. Tao, P. Wang, and H. Yang, Nucl. Phys. B,922: 346 (2017), arXiv:1505.03045[grqc
- [97]
S. Yang, J. Wan, J. Chenet al.,Weak cosmic censorship conjecture for the novel 4Dcharged Einstein-Gauss-Bonnet black hole with test scalar field and particle, arXiv: 2004.07934[gr-qc]